131 citations · 167 across the 3 of their papers we have counts for
4 papers
Early evolution of clumps formed via gravitational instability in protoplanetary disks; precursors of Hot Jupiters?
Marina Galvagni, Lucio Mayer
Although it is fairly established that Gravitational Instability (GI) should occur in the early phases of the evolution of a protoplanetary disk, the fate of the clumps resulting f…
Large grains can grow in circumstellar discs
Farzana Meru, Marina Galvagni, Christoph Olczak +1
We perform coagulation & fragmentation simulations to understand grain growth in T Tauri & brown dwarf discs. We present a physically-motivated approach using a probability distrib…
Growth of grains in Brown Dwarf disks
Farzana Meru, Marina Galvagni, Christoph Olczak
We perform coagulation and fragmentation simulations using the new physically-motivated model by Garaud et al. (2013) to determine growth locally in brown dwarf disks. We show that…
From dust to planetesimals: an improved model for collisional growth in protoplanetary disks
Pascale Garaud, Farzana Meru, Marina Galvagni +1
Planet formation occurs within the gas and dust rich environments of protoplanetary disks. Observations of these objects show that the growth of primordial sub micron sized particl…